SDO HMI 2014-08-06 12:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.16 | 19.96 | 2.37 | 14.94 | -21.38 | 157.12 | -40.71 | 125.83 | 0.7506 | 22.0 | 103.5 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.08 | 0.00 | 0.71 | -17.54 | 164.70 | -33.13 | 126.45 | 0.6502 | 648.0 | 503.1 | |
| 0.00 | 1.27 | 0.00 | 0.92 | -22.84 | 159.98 | -37.85 | 129.35 | 0.7336 | 592.0 | 453.8 | |
| 0.00 | 1.08 | 0.00 | 0.81 | -22.88 | 157.92 | -39.91 | 128.02 | 0.7526 | 256.0 | 273.7 | |
| 0.00 | 0.90 | 0.00 | 0.67 | -21.40 | 157.57 | -40.26 | 126.10 | 0.7469 | 392.0 | 422.6 | |
| 2.62 | 6.87 | 1.95 | 5.10 | -21.23 | 157.50 | -40.33 | 125.86 | 0.7466 | 590.0 | 478.8 | |
| 0.00 | 2.44 | 0.00 | 1.85 | -21.72 | 156.38 | -41.45 | 125.73 | 0.7599 | 416.0 | 274.8 | |
| 0.00 | 0.45 | 0.00 | 0.34 | -20.80 | 156.52 | -41.31 | 124.75 | 0.7533 | 367.0 | 320.8 | |
| 0.00 | 0.99 | 0.00 | 0.76 | -21.85 | 156.11 | -41.72 | 125.71 | 0.7630 | -241.0 | -215.5 | |
| 0.00 | 0.54 | 0.00 | 0.42 | -22.28 | 155.38 | -42.45 | 125.76 | 0.7720 | -495.0 | -509.7 | |
| 0.00 | 0.27 | 0.00 | 0.21 | -20.97 | 155.06 | -42.78 | 124.09 | 0.7680 | -546.0 | -426.0 | |
| 0.00 | 1.27 | 0.00 | 0.98 | -21.50 | 154.82 | -43.01 | 124.56 | 0.7729 | -684.0 | -670.8 | |
| 0.54 | 1.90 | 0.42 | 1.47 | -21.17 | 154.76 | -43.07 | 124.14 | 0.7717 | -745.2 | -608.9 | |
| 0.00 | 0.90 | 0.00 | 0.70 | -21.34 | 154.70 | -43.13 | 124.30 | 0.7732 | -481.0 | -479.2 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |